Gliese 754

Gliese 754 is a red dwarf star of spectral type M4.5V in the constellation Telescopium.[1] It has an apparent magnitude of 12.23 and is around 19.3 light-years distant.[1] It is one of the hundred closest stars to the Solar System. Calculations of its orbit around the Milky Way showed that it was eccentric, and indicate that it might be a thick disk object.[2]

GJ 754
Observation data
Epoch J2000      Equinox J2000
Constellation Telescopium
Right ascension  19h 20m 47.955s [1]
Declination −45° 33′ 28.33″ [1]
Characteristics
Spectral type M4.5V[1]
Database references
SIMBADdata

Planetary System

In June 2019 one planet candidate were reported in orbit around Gliese 754. [3]

The Gliese 754 planetary system
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b 9.8+4.6
−5.2 M⊕		 0.277+0.025
−0.028		 78.37+0.55
−0.47		 0.03+0.20
−0.03		 — —
gollark: For all that tailscale fairly good it is probably not ideal on *really* resource-constrained systems.
gollark: (it does not run any software except tailscale and sshd)
gollark: (30MB of which is tailscale)
gollark: Anyway, Alpine is quite minimal, I think. All the processes conveniently fit onto my screen in htop (half are just tailscale ones), and it's using 52MB of memory.
gollark: (Pis before the Raspberry Pi 3 *do not* exist.)

References
  1. "LHS 60 -- High proper-motion Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 4 July 2014.
  2. Innanen, K.A.; Flynn, C. (2010). "The Radial Velocity, Space Motion, and Galactic Orbit of GJ 754". Journal of the Royal Astronomical Society of Canada. 104 (6): 223–24. Bibcode:2010JRASC.104..223I.
  3. Barnes, J. R.; et al. (2019-06-11). "Frequency of planets orbiting M dwarfs in the Solar neighbourhood". arXiv:1906.04644.
  • Jao, Wei-Chun; Henry, Todd J.; Subasavage, John P.; Brown, Misty A.; Ianna, Philip A.; Bartlett, Jennifer L.; Costa, Edgardo; Méndez, René A. (2005). "The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with mu >= 1.0" yr-1 (MOTION Sample)". The Astronomical Journal. 129 (4): 1954–1967. arXiv:astro-ph/0502167. Bibcode:2005AJ....129.1954J. doi:10.1086/428489.


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